Nonclassical light

Nonclassical light is light that cannot be described using classical electromagnetism; its characteristics are described by the quantized electromagnetic field and quantum mechanics. Nonclassical light has nonclassical noise properties called quantum noise, which can be understood on the basis of quantum optics.

Most common described forms of nonclassical light are the following:

Glauber–Sudarshan P representation

It has been shown that the density matrix for any state of light can be written as:

\widehat{\rho} = \int \varphi(\alpha) |{\alpha}\rangle \langle {\alpha}| \rm{d}^2 \alpha,

where \scriptstyle|\alpha\rangle is a coherent state. A classical state of light is one in which \scriptstyle\varphi(\alpha) \, is a probability density function. If it is not, the state is said to be nonclassical.[1]

Aspects of \scriptstyle \varphi(\alpha) \, that would make it nonclassical are:

The matter is not quite simple. According to Mandel and Wolf: "The different coherent states are not [mutually] orthogonal, so that even if \scriptstyle P(\alpha) \, behaved like a true probability density [function], it would not describe probabilities of mutually exclusive states."[1]

References

Citations

Citation bibliography

Mandel, L.; Wolf, E. (1995), Optical Coherence and Quantum Optics, Cambridge UK: Cambridge University Press, ISBN 0-521-41711-2 

General references

External links


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